{
  "annotation_id": "df3c960b-3ce3-4ee0-ab5b-e771bb039b3f",
  "date_created": "2026-03-02T18:00:00.536000Z",
  "date_modified": "2026-03-02T18:00:00.536000Z",
  "file_hash": "803a51e71eebc8c5f05d00af3552cd25bbcec27d5db727ee295e31f01fd15d18",
  "private": false,
  "record": {
    "abstract": "Available Skyrme parametrizations with hyperons are examined from the point\nof view of their suitability for applications to neutron stars. It is shown\nthat the hyperons can attenuate or even remove the problem of ferromagnetic\ninstability common to (nearly) all Skyrme parametrizations of the\nnucleon-nucleon interaction. At high density the results are very sensitive to\nthe choice of the Lambda-Lambda interaction. The selected parameter sets are\nthen used to obtain the resulting properties of both cold neutron stars and hot\nprotoneutron stars. The general features known from other models are recovered.",
    "arxiv_id": "nucl-th/0407083",
    "authors": [
      "L. Mornas"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1140/epja/i2004-10142-5",
    "journal_ref": "Eur.Phys.J. A24 (2005) 293-312",
    "title": "Neutron stars in a Skyrme model with hyperons",
    "url": "https://arxiv.org/abs/nucl-th/0407083"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "d9413efd-ac0d-4d4a-8cca-7968d5a1168f",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}